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dc.contributor.author양종만-
dc.date.accessioned2016-08-27T02:08:47Z-
dc.date.available2016-08-27T02:08:47Z-
dc.date.issued2003-
dc.identifier.issn0374-4884-
dc.identifier.otherOAK-1360-
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/215567-
dc.description.abstractWe review several models of continuum mechanics of interstellar media with different gas-dust composition which are utilized in current theoretical interpretation of Zeeman measurements of the molecular linewidths detected from star-forming interstellar clouds. Emphasis is placed on wave motions attributed to the presence in the interstellar medium of the Galactic magnetic field.-
dc.languageEnglish-
dc.publisherKOREAN PHYSICAL SOC-
dc.subjectinterstellar medium-
dc.subjectmagnetic fields-
dc.titleLarge scale wave dynamics of interstellar medium in galactic magnetic fields-
dc.typeArticle-
dc.typeProceedings Paper-
dc.relation.volume42-
dc.relation.indexSCI-
dc.relation.indexSCIE-
dc.relation.indexSCOPUS-
dc.relation.indexKCI-
dc.relation.startpageS73-
dc.relation.lastpageS77-
dc.relation.journaltitleJOURNAL OF THE KOREAN PHYSICAL SOCIETY-
dc.identifier.wosidWOS:000181168200012-
dc.identifier.scopusid2-s2.0-0037309194-
dc.author.googleBastrukov, S-
dc.author.googleYang, JM-
dc.contributor.scopusid양종만(15039320200;8833888100)-
dc.date.modifydate20220119163221-
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자연과학대학 > 물리학전공 > Journal papers
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